E. J. Salumbides

activity

20142021

most citedLimits on a Gravitational Field Dependence of the Proton--Electron Mass Ratio from H

_{2}

in White Dwarf Stars

31 citations · 93 across the 9 of their papers we have counts for

collaborators

Showing 2014Show all

3 papers · 1 filter

physics.atom-ph2014★ 20 cited

H $_{2}$ Lyman and Werner band lines and their sensitivity for a variation of the proton-electron mass ratio in the gravitational potential of white dwarfs

E. J. Salumbides, J. Bagdonaite, H. Abgrall +2

Recently an accurate analysis of absorption spectra of molecular hydrogen, observed with the Cosmic Origins Spectrograph aboard the Hubble Space Telescope, in the photosphere of wh…

physics.atom-ph2014★ 4 cited

$B^{1} Σ_{u}^{+}$ and $E F^{1} Σ_{g}^{+}$ level energies of D $_{2}$

E. J. Salumbides, D. Bailly, M. Vervloet +1

Accurate absolute level energies of the $B^{1} Σ_{u}^{+}$ , $v = 0 - 8, N$ and $E F^{1} Σ_{g}^{+}$ , $v = 0 - 21, N$ rovibrational quantum states of molecular deuterium are derived by combini…

gr-qc2014★ 31 cited

Limits on a Gravitational Field Dependence of the Proton--Electron Mass Ratio from H $_{2}$ in White Dwarf Stars

Julija Bagdonaite, Edcel J. Salumbides, Simon P. Preval +4

Spectra of molecular hydrogen (H $_{2}$ ) are employed to search for a possible proton-to-electron mass ratio ( $μ$ ) dependence on gravity. The Lyman transitions of H $_{2}$ , observed with…

H2​ Lyman and Werner band lines and their sensitivity for a variation of the proton-electron mass ratio in the gravitational potential of white dwarfs

B1Σu+​ and EF1Σg+​ level energies of D2​

Limits on a Gravitational Field Dependence of the Proton--Electron Mass Ratio from H2​ in White Dwarf Stars

H $_{2}$ Lyman and Werner band lines and their sensitivity for a variation of the proton-electron mass ratio in the gravitational potential of white dwarfs

$B^{1} Σ_{u}^{+}$ and $E F^{1} Σ_{g}^{+}$ level energies of D $_{2}$

Limits on a Gravitational Field Dependence of the Proton--Electron Mass Ratio from H $_{2}$ in White Dwarf Stars